Description:I will discuss a new class of solutions to the Cosmological Constant and Higgs fine-tuning problems that do not require the presence of new physics at the Large Hadron Collider. Instead, they involve a new proposal for the history of the universe wherein these parameters achieve their observed values as a result of cosmic evolution. In addition, I will exploit a loop-hole in the singularity theorems of General Relativity to allow for a calculable, non-singular 'bounce', essential for a solution to the cosmological constant problem. (2:00 PM, 726 Broadway, 940, CCPP Seminar)